New CAST limit on the axion–photon interaction

V. Anastassopoulos; S.  Aune; K. Barth; A. Belov; H. Bräuninger; G. Cantatore; J. M. Carmona; J. F.  Castel; S. A.  Cetin; Finn Erland Christensen; J. I.  Collar; T. Dafni; M. Davenport; T. A. Decker; A. Dermenev; K. Desch; C. Eleftheriadis; G. Fanourakis; E. Ferrer-Ribas; H. Fischer; J. A. García; A.  Gardikiotis; J. G.  Garza; E. N.  Gazis; T. Geralis; I Giomataris; S. Gninenko; C. J. Hailey; M. D.  Hasinoff; D H H Hoffmann; F. J.  Iguaz; I G Irastorza; A.  Jakobsen; J.  Jacoby; K Jakovčić; J Kaminski; M. Karuza; N. Kralj; M Krčmar; S.  Kostoglou; Ch.  Krieger; B Lakić; J. M. Laurent; A.  Liolios; A.  Ljubicic; G.  Luzón; M.  Maroudas; L.  Miceli; S.  Neff; I.  Ortega; T Papaevangelou; K.  Paraschou; M. J. Pivovaro; G Raffelt; M.  Rosu; J Ruz; E.  Ruiz Chóliz; I Savvidis; S.  Schmidt; Y. K. Semertzidis; S. K.  Solanki; L.  Stewart; T Vafeiadis; J. K. Vogel; S. C. Yildiz; K Zioutas

doi:10.1038/NPHYS4109

New CAST limit on the axion–photon interaction

V. Anastassopoulos
, S. Aune
, K. Barth
, A. Belov
, H. Bräuninger
, G. Cantatore
, J. M. Carmona
, J. F. Castel
, S. A. Cetin
, Finn Erland Christensen
, J. I. Collar
, T. Dafni
, M. Davenport
, T. A. Decker
, A. Dermenev
, K. Desch
, C. Eleftheriadis
, G. Fanourakis
, E. Ferrer-Ribas
, H. Fischer

J. A. García, A. Gardikiotis, J. G. Garza, E. N. Gazis, T. Geralis, I Giomataris, S. Gninenko, C. J. Hailey, M. D. Hasinoff, D H H Hoffmann, F. J. Iguaz, I G Irastorza, A. Jakobsen, J. Jacoby, K Jakovčić, J Kaminski, M. Karuza, N. Kralj, M Krčmar, S. Kostoglou, Ch. Krieger, B Lakić, J. M. Laurent, A. Liolios, A. Ljubicic, G. Luzón, M. Maroudas, L. Miceli, S. Neff, I. Ortega, T Papaevangelou, K. Paraschou, M. J. Pivovaro, G Raffelt, M. Rosu, J Ruz, E. Ruiz Chóliz, I Savvidis, S. Schmidt, Y. K. Semertzidis, S. K. Solanki, L. Stewart, T Vafeiadis, J. K. Vogel, S. C. Yildiz, K Zioutas

Istanbul Bilgi University
University of Patras
Centre d'Etudes Nucléaires de Saclay
CERN
Russian Academy of Sciences
Max Planck Institute
University of Trieste
University of Zaragoza
Lawrence Livermore National Laboratory
University of Bonn
University of Freiburg
The University of Chicago
Aristotle University of Thessaloniki
Demokritos National Centre for Scientific Research
University of British Columbia
Technical University of Denmark
French Alternative Energies and Atomic Energy Commission
Columbia University
Technische Universität Darmstadt
Rudjer Boskovic Institute
Rheinische Friedrich-Wilhelms-Universität Bonn
Dogus University
Johann Wolfgang Goethe-Universität Frankfurt
University of Rijeka
Institute for Basic Science
Max Planck Institute for Solar System Research
National Technical University of Athens

Research output: Contribution to journal › Journal article › Research › peer-review

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Abstract

Hypothetical low-mass particles, such as axions, provide a compelling explanation for the dark matter in the universe. Suchparticles are expected to emerge abundantly from the hot interior of stars. To test this prediction, the CERN Axion SolarTelescope (CAST) uses a 9 T refurbished Large Hadron Collider test magnet directed towards the Sun. In the strong magneticfield, solar axions can be converted to X-ray photons which can be recorded by X-ray detectors. In the 2013–2015 run, thanksto low-background detectors and a new X-ray telescope, the signal-to-noise ratio was increased by about a factor of three.Here, we report the best limit on the axion–photon coupling strength (0.66x10^-10GeV^-1 at 95% confidence level) set byCAST, which now reaches similar levels to the most restrictive astrophysical bounds.

Original language	English
Journal	Nature Physics
Volume	13
Pages (from-to)	584-591
ISSN	1745-2473
DOIs	https://doi.org/10.1038/NPHYS4109
Publication status	Published - 2017

Bibliographical note

This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

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Anastassopoulos, V., Aune, S., Barth, K., Belov, A., Bräuninger, H., Cantatore, G., Carmona, J. M., Castel, J. F., Cetin, S. A., Christensen, F. E., Collar, J. I., Dafni, T., Davenport, M., Decker, T. A., Dermenev, A., Desch, K., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., ... Zioutas, K. (2017). New CAST limit on the axion–photon interaction. Nature Physics, 13, 584-591. https://doi.org/10.1038/NPHYS4109

@article{3ed9885580b942939f2003c071235052,

title = "New CAST limit on the axion{\textendash}photon interaction",

abstract = "Hypothetical low-mass particles, such as axions, provide a compelling explanation for the dark matter in the universe. Suchparticles are expected to emerge abundantly from the hot interior of stars. To test this prediction, the CERN Axion SolarTelescope (CAST) uses a 9 T refurbished Large Hadron Collider test magnet directed towards the Sun. In the strong magneticfield, solar axions can be converted to X-ray photons which can be recorded by X-ray detectors. In the 2013{\textendash}2015 run, thanksto low-background detectors and a new X-ray telescope, the signal-to-noise ratio was increased by about a factor of three.Here, we report the best limit on the axion{\textendash}photon coupling strength (0.66x10-10 GeV-1 at 95\% confidence level) set byCAST, which now reaches similar levels to the most restrictive astrophysical bounds.",

author = "V. Anastassopoulos and S. Aune and K. Barth and A. Belov and H. Br{\"a}uninger and G. Cantatore and Carmona, \{J. M.\} and Castel, \{J. F.\} and Cetin, \{S. A.\} and Christensen, \{Finn Erland\} and Collar, \{J. I.\} and T. Dafni and M. Davenport and Decker, \{T. A.\} and A. Dermenev and K. Desch and C. Eleftheriadis and G. Fanourakis and E. Ferrer-Ribas and H. Fischer and Garc{\'i}a, \{J. A.\} and A. Gardikiotis and Garza, \{J. G.\} and Gazis, \{E. N.\} and T. Geralis and I Giomataris and S. Gninenko and Hailey, \{C. J.\} and Hasinoff, \{M. D.\} and Hoffmann, \{D H H\} and Iguaz, \{F. J.\} and Irastorza, \{I G\} and A. Jakobsen and J. Jacoby and K Jakov{\v c}i{\'c} and J Kaminski and M. Karuza and N. Kralj and M Kr{\v c}mar and S. Kostoglou and Ch. Krieger and B Laki{\'c} and Laurent, \{J. M.\} and A. Liolios and A. Ljubicic and G. Luz{\'o}n and M. Maroudas and L. Miceli and S. Neff and I. Ortega and T Papaevangelou and K. Paraschou and Pivovaro, \{M. J.\} and G Raffelt and M. Rosu and J Ruz and \{Ruiz Ch{\'o}liz\}, E. and I Savvidis and S. Schmidt and Semertzidis, \{Y. K.\} and Solanki, \{S. K.\} and L. Stewart and T Vafeiadis and Vogel, \{J. K.\} and Yildiz, \{S. C.\} and K Zioutas",

note = "This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.",

year = "2017",

doi = "10.1038/NPHYS4109",

language = "English",

volume = "13",

pages = "584--591",

journal = "Nature Physics",

issn = "1745-2473",

publisher = "Nature Research",

}

Anastassopoulos, V, Aune, S, Barth, K, Belov, A, Bräuninger, H, Cantatore, G, Carmona, JM, Castel, JF, Cetin, SA, Christensen, FE, Collar, JI, Dafni, T, Davenport, M, Decker, TA, Dermenev, A, Desch, K, Eleftheriadis, C, Fanourakis, G, Ferrer-Ribas, E, Fischer, H, García, JA, Gardikiotis, A, Garza, JG, Gazis, EN, Geralis, T, Giomataris, I, Gninenko, S, Hailey, CJ, Hasinoff, MD, Hoffmann, DHH, Iguaz, FJ, Irastorza, IG, Jakobsen, A, Jacoby, J, Jakovčić, K, Kaminski, J, Karuza, M, Kralj, N, Krčmar, M, Kostoglou, S, Krieger, C, Lakić, B, Laurent, JM, Liolios, A, Ljubicic, A, Luzón, G, Maroudas, M, Miceli, L, Neff, S, Ortega, I, Papaevangelou, T, Paraschou, K, Pivovaro, MJ, Raffelt, G, Rosu, M, Ruz, J, Ruiz Chóliz, E, Savvidis, I, Schmidt, S, Semertzidis, YK, Solanki, SK, Stewart, L, Vafeiadis, T, Vogel, JK, Yildiz, SC & Zioutas, K 2017, 'New CAST limit on the axion–photon interaction', Nature Physics, vol. 13, pp. 584-591. https://doi.org/10.1038/NPHYS4109

TY - JOUR

T1 - New CAST limit on the axion–photon interaction

AU - Anastassopoulos, V.

AU - Aune, S.

AU - Barth, K.

AU - Belov, A.

AU - Bräuninger, H.

AU - Cantatore, G.

AU - Carmona, J. M.

AU - Castel, J. F.

AU - Cetin, S. A.

AU - Christensen, Finn Erland

AU - Collar, J. I.

AU - Dafni, T.

AU - Davenport, M.

AU - Decker, T. A.

AU - Dermenev, A.

AU - Desch, K.

AU - Eleftheriadis, C.

AU - Fanourakis, G.

AU - Ferrer-Ribas, E.

AU - Fischer, H.

AU - García, J. A.

AU - Gardikiotis, A.

AU - Garza, J. G.

AU - Gazis, E. N.

AU - Geralis, T.

AU - Giomataris, I

AU - Gninenko, S.

AU - Hailey, C. J.

AU - Hasinoff, M. D.

AU - Hoffmann, D H H

AU - Iguaz, F. J.

AU - Irastorza, I G

AU - Jakobsen, A.

AU - Jacoby, J.

AU - Jakovčić, K

AU - Kaminski, J

AU - Karuza, M.

AU - Kralj, N.

AU - Krčmar, M

AU - Kostoglou, S.

AU - Krieger, Ch.

AU - Lakić, B

AU - Laurent, J. M.

AU - Liolios, A.

AU - Ljubicic, A.

AU - Luzón, G.

AU - Maroudas, M.

AU - Miceli, L.

AU - Neff, S.

AU - Ortega, I.

AU - Papaevangelou, T

AU - Paraschou, K.

AU - Pivovaro, M. J.

AU - Raffelt, G

AU - Rosu, M.

AU - Ruz, J

AU - Ruiz Chóliz, E.

AU - Savvidis, I

AU - Schmidt, S.

AU - Semertzidis, Y. K.

AU - Solanki, S. K.

AU - Stewart, L.

AU - Vafeiadis, T

AU - Vogel, J. K.

AU - Yildiz, S. C.

AU - Zioutas, K

N1 - This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

PY - 2017

Y1 - 2017

N2 - Hypothetical low-mass particles, such as axions, provide a compelling explanation for the dark matter in the universe. Suchparticles are expected to emerge abundantly from the hot interior of stars. To test this prediction, the CERN Axion SolarTelescope (CAST) uses a 9 T refurbished Large Hadron Collider test magnet directed towards the Sun. In the strong magneticfield, solar axions can be converted to X-ray photons which can be recorded by X-ray detectors. In the 2013–2015 run, thanksto low-background detectors and a new X-ray telescope, the signal-to-noise ratio was increased by about a factor of three.Here, we report the best limit on the axion–photon coupling strength (0.66x10-10 GeV-1 at 95% confidence level) set byCAST, which now reaches similar levels to the most restrictive astrophysical bounds.

AB - Hypothetical low-mass particles, such as axions, provide a compelling explanation for the dark matter in the universe. Suchparticles are expected to emerge abundantly from the hot interior of stars. To test this prediction, the CERN Axion SolarTelescope (CAST) uses a 9 T refurbished Large Hadron Collider test magnet directed towards the Sun. In the strong magneticfield, solar axions can be converted to X-ray photons which can be recorded by X-ray detectors. In the 2013–2015 run, thanksto low-background detectors and a new X-ray telescope, the signal-to-noise ratio was increased by about a factor of three.Here, we report the best limit on the axion–photon coupling strength (0.66x10-10 GeV-1 at 95% confidence level) set byCAST, which now reaches similar levels to the most restrictive astrophysical bounds.

U2 - 10.1038/NPHYS4109

DO - 10.1038/NPHYS4109

M3 - Journal article

SN - 1745-2473

VL - 13

SP - 584

EP - 591

JO - Nature Physics

JF - Nature Physics

ER -

New CAST limit on the axion–photon interaction

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